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THE LOIANO CAMPAIGNS FOR PHOTOMETRY AND SPECTROSCOPY OF GEOSYNCHRONOUS OBJECTS

机译:用于对地物的光度法和光谱法的Loiano摄影机

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A pilot program for the physical characterization of the space debris population in high Earth orbits was started at the152cm G.D. Cassini Telescope in Loiano, operated by the INAF Astronomical Observatory of Bologna, Italy. TheRitchey - Chretien optical system has is equipped with BFOSC (Bologna Faint Object Spectrograph and Camera), amultipurpose instrument for imaging and spectroscopy, with an EEV CCD (1340x1300 px).Several BVRI photometric images of active satellites, disposed spacecraft and upper stages were acquired during onenight in February 2011 and three nights in August 2011. Of course, a number of photometric calibration fields andSolar analogue stars (spectral standards) were observed for calibration purposes.A few High Area to Mass Ratio, HAMR, objects were observed and lightcurves were obtained for them.The paper presents the obtained data and the discussion on how to establish the physical nature and hence, possibly,the origin of the targets.
机译:在高地球轨道上开始了一项对高地球轨道上的空间碎片种群进行物理表征的试点计划。 152厘米长的洛里亚诺G.D.卡西尼望远镜,由意大利博洛尼亚的INAF天文台操作。这 Ritchey-Chretien光学系统配备了BFOSC(博洛尼亚微弱物体光谱仪和照相机), 具有EEV CCD(1340x1300 px)的用于成像和光谱学的多功能仪器。 在一次地震中,获得了几个活动卫星,已放置的航天器和高层的BVRI光度图像 2011年2月的晚上和2011年8月的三个晚上。 观测太阳模拟星(光谱标准)以进行校准。 观察到一些高面积质量比HAMR,并获得了它们的光曲线。 本文介绍了获得的数据,并讨论了如何建立物理性质,因此,有可能 目标的来源。

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